Abstract <p>The astrophysical experiment TAIGA-10 (Tunka Advanced Instrument for cosmic ray physics and Gamma-ray Astronomy) is planned to extend by mounting new telescopes with improved parameters: a smaller camera pixel size of a larger mirror diameter. The simulation of new and already installed telescopes has been conducted, and expected improvement in the hadron background rejection after transition to smaller pixel sizes and a larger mirror diameter has been quantitatively estimated.</p>

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Hadron Rejection in an Imaging Air Cherenkov Telescope Depending on the Mirror Diameter and Camera Pixel Size

  • E. B. Postnikov,
  • I. I. Astapov,
  • P. A. Bez’’yazykov,
  • A. V. Blinov,
  • E. A. Bonvech,
  • A. N. Borodin,
  • N. M. Budnev,
  • A. V. Bulan,
  • D. V. Chernov,
  • A. Chiavassa,
  • A. N. Dyachok,
  • A. R. Gafarov,
  • A. Yu. Garmash,
  • V. M. Grebenyuk,
  • E. O. Gres’,
  • O. A. Gres’,
  • T. I. Gres’,
  • A. A. Grinyuk,
  • O. G. Grishin,
  • A. D. Ivanova,
  • A. L. Ivanova,
  • M. A. Ilyushin,
  • N. N. Kalmykov,
  • V. V. Kindin,
  • S. N. Kiryukhin,
  • R. P. Kokoulin,
  • N. I. Kolosov,
  • K. G. Kompaniets,
  • E. E. Korosteleva,
  • V. A. Kozhin,
  • E. A. Kravchenko,
  • A. P. Kryukov,
  • L. A. Kuzmichev,
  • A. A. Lagutin,
  • M. V. Lavrova,
  • Yu. E. Lemeshev,
  • B. K. Lubsandorzhiev,
  • N. B. Lubsandorzhiev,
  • A. D. Lukanov,
  • S. D. Malakhov,
  • R. R. Mirgazov,
  • R. D. Monkhoev,
  • E. A. Okuneva,
  • E. A. Osipova,
  • A. L. Pakhorukov,
  • A. Pan,
  • A. D. Panov,
  • L. V. Pankov,
  • A. A. Petrukhin,
  • I. A. Poddubnyi,
  • D. A. Podgrudkov,
  • E. G. Popova,
  • V. V. Prosin,
  • V. S. Ptuskin,
  • A. A. Pushnin,
  • R. I. Raikin,
  • A. V. Razumov,
  • E. V. Ryabov,
  • G. I. Rubtsov,
  • V. S. Samoliga,
  • I. Satyshev,
  • A. V. Shaykovskiy,
  • A. Yu. Sidorenkov,
  • A. A. Silaev,
  • A. A. Silaev Jr.,
  • A. V. Skurikhin,
  • A. V. Sokolov,
  • L. G. Sveshikova,
  • V. A. Tabolenko,
  • A. B. Tanaev,
  • M. Yu. Ternovoy,
  • L. G. Tkachev,
  • N. A. Ushakov,
  • P. A. Volchugov,
  • N. V. Volkov,
  • D. M. Voronin,
  • I. I. Yashin,
  • A. V. Zagorodnikov,
  • D. P. Zhurov,
  • V. N. Zirakashvili

摘要

Abstract

The astrophysical experiment TAIGA-10 (Tunka Advanced Instrument for cosmic ray physics and Gamma-ray Astronomy) is planned to extend by mounting new telescopes with improved parameters: a smaller camera pixel size of a larger mirror diameter. The simulation of new and already installed telescopes has been conducted, and expected improvement in the hadron background rejection after transition to smaller pixel sizes and a larger mirror diameter has been quantitatively estimated.